output
20062025
most citedSMILEI: a collaborative, open-source, multi-purpose particle-in-cell code for plasma simulation

580 citations

Showing 2016Show all

16 papers · 1 filter

hep-lat2016★ 40 cited

Slope and curvature of the hadron vacuum polarization at vanishing virtuality from lattice QCD

Sz. Borsanyi, Z. Fodor, T. Kawanai +7

We compute the slope and curvature, at vanishing four-momentum transfer squared, of the leading order hadron vacuum polarization function, using lattice QCD. Calculations are perfo…

astro-ph.EP2016★ 132 cited

Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models

David S. Amundsen, Pascal Tremblin, James Manners +2

The correlated-k method is frequently used to speed up radiation calculations in both one-dimensional and three-dimensional atmosphere models. An inherent difficulty with this meth…

astro-ph.EP2016★ 112 cited

The UK Met Office GCM with a sophisticated radiation scheme applied to the hot Jupiter HD 209458b

David S. Amundsen, Nathan J. Mayne, Isabelle Baraffe +6

To study the complexity of hot Jupiter atmospheres revealed by observations of increasing quality, we have adapted the UK Met Office global circulation model (GCM), the Unified Mod…

math.NA2016★ 3 cited

Sharpening methods for finite volume schemes

B Després, S Kokh, Frédéric Lagoutière

We review sharpening methods for finite volume schemes, with an emphasis on the basic structure of sharpening methods. It covers high order methods and non linear techniques for li…

physics.flu-dyn2016★ 15 cited

A hierarchy of simple hyperbolic two-fluid models for bubbly flows

Florence Drui, Adam Larat, Samuel Kokh +1

With the objective of modeling both separate and disperse two-phase flows, we use in this paper a methodology for deriving two-fluid models that do not assume any flow topology. Th…

astro-ph.GA2016★ 93 cited

Feedback in Clouds II: UV Photoionisation and the first supernova in a massive cloud

Sam Geen, Patrick Hennebelle, Pascal Tremblin +1

Molecular cloud structure is regulated by stellar feedback in various forms. Two of the most important feedback processes are UV photoionisation and supernovae from massive stars.…